Abstract. The pion mass difference generates a pronounced cusp in the π 0 π 0 invariant mass distribution of K + → π 0 π 0 π + decays. As originally pointed out by Cabibbo, an accurate measurement of the cusp may allow one to pin down the S-wave pion-pion scattering lengths to high precision. We present the non-relativistic effective field theory framework that permits to determine the structure of this cusp in a straightforward manner, including the effects of radiative corrections. Applications of the same formalism to other decay channels, in particular η and η ′ decays, are also discussed.
The pion mass and pion-pion scatteringThe approximate chiral symmetry of the strong interactions severely constrains the properties and interactions of the lightest hadronic degrees of freedom, the would-be Goldstone bosons (in the chiral limit of vanishing quark masses) of spontaneous chiral symmetry breaking that can be identified with the pions. The effective field theory that systematically exploits all the consequences that can be derived from symmetries is chiral perturbation theory [1,2], which provides an expansion of low-energy observables in terms of small quark masses and small momenta. One of the most elementary consequences of chiral symmetry is the well-known Gell-Mann-Oakes-Renner relation [3] for the pion mass M in terms of the light quark masses (at leading order),A non-vanishing order parameter B, related to the light quark condensate via the pion decay constant F (in the chiral limit), is a sufficient (but not necessary) condition for chiral symmetry breaking. Chiral perturbation theory allows to calculate corrections to this relation [2],with the a priori unknown low-energy constantl 3 . Another way to write Eq. (2) is thereforeand the natural question arises: how do we know that the leading term in the quark-mass expansion of M 2 π really dominates the series?l 3 could actually be anomalously large, the consequence of which has been explored as an a e-mail: kubis@hiskp.uni-bonn.de alternative scenario of chiral symmetry breaking under the name of generalized chiral perturbation theory [4].Fortunately, chiral low-energy constants tend to appear in more than one observable, and indeed,l 3 also features in the next-to-leading-order corrections to the isospin I = 0 S-wave pion-pion scattering length a do not depend on the D-wave scattering lengths as input, but rather yield values for all ππ threshold parameters as results. The predictions Eq. (6) are among the most precise in